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http://eprints.org/relation/isVersionOf http://eprints.iliauni.edu.ge/id/document/2835 http://eprints.org/relation/isVolatileVersionOf http://eprints.iliauni.edu.ge/id/document/2835 http://eprints.org/relation/issmallThumbnailVersionOf http://eprints.iliauni.edu.ge/id/document/2835 archive 131 disk0/00/00/07/32 2014-01-30 12:35:31 2015-03-27 07:02:14 2014-01-30 12:35:31 article show Gogoberidze Grigol Kahniashvili Tina tinatin@iliauni.edu.ge Kosowsky Arthur pub QC public Energy injection into the early universe can induce turbulent motions of the primordial plasma, which in turn act as a source for gravitational radiation. Earlier work computed the amplitude and characteristic frequency of the relic gravitational wave background, as a function of the total energy injected and the stirring scale of the turbulence. This paper computes the frequency spectrum of relic gravitational radiation from a turbulent source of the stationary Kolmogoroff form which acts for a given duration, making no other approximations. We also show that the limit of long source wavelengths, commonly employed in aeroacoustic problems, is an excellent approximation. The gravitational waves from cosmological turbulence around the electroweak energy scale will be detectable by future space-based laser interferometers for a substantial range of turbulence parameters. 2007 published Spectrum of gravitational radiation from primordial turbulence 76 083002 TRUE